Interhemispheric differences of mesosphere-lower thermosphere winds and tides investigated from three whole-atmosphere models and meteor radar observations

Stober, G.; Kuchar, A.; Pokhotelov, D.; Liu, H.; Liu, H.-L.; Schmidt, H.; Jacobi, C.; Baumgarten, K.; Brown, P.; Janches, D.; Murphy, D.; Kozlovsky, A.; Lester, M.; Belova, E.; Kero, J.; Mitchell, N.. 2021 Interhemispheric differences of mesosphere-lower thermosphere winds and tides investigated from three whole-atmosphere models and meteor radar observations. Atmospheric Chemistry and Physics, 21 (18). 13855-13902. 10.5194/acp-21-13855-2021

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Official URL: https://acp.copernicus.org/articles/21/13855/2021/

Abstract/Summary

Long-term and continuous observations of mesospheric-lower thermospheric winds are rare, but they are important to investigate climatological changes at these altitudes on timescales of several years, covering a solar cycle and longer. Such long time series are a natural heritage of the mesosphere-lower thermosphere climate, and they are valuable to compare climate models or long-term runs of general circulation models (GCMs). Here we present a climatological comparison of wind observations from six meteor radars at two conjugate latitudes to validate the corresponding mean winds and atmospheric diurnal and semidiurnal tides from three GCMs, namely the Ground-to-Topside Model of Atmosphere and Ionosphere for Aeronomy (GAIA), the Whole Atmosphere Community Climate Model Extension (Specified Dynamics) (WACCM-X(SD)), and the Upper Atmosphere ICOsahedral Non-hydrostatic (UA-ICON) model. Our results indicate that there are interhemispheric differences in the seasonal characteristics of the diurnal and semidiurnal tide. There are also some differences in the mean wind climatologies of the models and the observations. Our results indicate that GAIA shows reasonable agreement with the meteor radar observations during the winter season, whereas WACCM-X(SD) shows better agreement with the radars for the hemispheric zonal summer wind reversal, which is more consistent with the meteor radar observations. The free-running UA-ICON tends to show similar winds and tides compared to WACCM-X(SD).

Item Type:	Publication - Article
Digital Object Identifier (DOI):	10.5194/acp-21-13855-2021
ISSN:	1680-7316
Date made live:	27 Sep 2021 09:17 +0 (UTC)
URI:	https://nora.nerc.ac.uk/id/eprint/531106

Item Type:

Publication - Article

Digital Object Identifier (DOI):

10.5194/acp-21-13855-2021

ISSN:

1680-7316

Date made live:

27 Sep 2021 09:17 +0 (UTC)

URI:

https://nora.nerc.ac.uk/id/eprint/531106